A single CNN trained on one 150 Hz frequency band detects hour-to-day neutron star transient signals across bands with sensitivity comparable to the Generalized FrequencyHough, and was applied to real LIGO data from the GW170817 remnant search.
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How effective is machine learning to detect long transient gravitational waves from neutron stars in a real search?
A single CNN trained on one 150 Hz frequency band detects hour-to-day neutron star transient signals across bands with sensitivity comparable to the Generalized FrequencyHough, and was applied to real LIGO data from the GW170817 remnant search.